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Gaussian CMB

WMAP-Constrained CMB Realisation

Carlo Baccigalupi and Mark Ashdown

Gaussian CMB realisation (temperature and polarisation) with the temperature (T) part constrained using WMAP ILC map at multipoles l <= 70, available here. The TT, TE and EE power spectra used to generate the rest of the multipoles are those predicted by the best-fit cosmological model, also hosted at the website above, without running spectral index. The part of the E signal which is correlated with T was simulated to provide the predicted amount of TE power, within cosmic variance.

The template, together with the codes and files to produce it, can be found here or here

   
last update for this page: 2005-10-28 21:19:27
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